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Modeling the galaxy/light-mass connection with cosmological simulations

I review some results on the galaxy/light-mass connection obtained by dissipationless simulations in combination with a simple, non-parametric model to connect halo circular velocity to the luminosity of the galaxy they would host. I focus on the galaxy-mass correlation and mass-to-light ratios obtained from galaxy up to cluster scales. The predictions of this simple scheme are shown to be in very good agreement with SDSS observations.

preprint2006arXivOpen access
Argyro Tasitsiomi
astro-ph
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Argyro Tasitsiomi

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